翻訳と辞書
Words near each other
・ Sabina-Francesca Foisor
・ Sabinada
・ Sabinaite
・ Sabinal
・ Sabinal Independent School District
・ Sabinal River
・ Sabinal, Texas
・ Sabinas
・ Sabinas brittle hair syndrome
・ Sabinas Hidalgo River
・ Sabinas Hidalgo, Nuevo León
・ Sabinas Municipality
・ Sabinas River
・ Sabinas, Coahuila
・ Sabindra Shrestha
Sabine (crater)
・ Sabine (disambiguation)
・ Sabine (given name)
・ Sabine (surname)
・ Sabine (TV series)
・ Sabine Andresen
・ Sabine Appelmans
・ Sabine Auken
・ Sabine Azéma
・ Sabine Baeß
・ Sabine Bank Light
・ Sabine Baring-Gould
・ Sabine baronets
・ Sabine Bau
・ Sabine Bay


Dictionary Lists
翻訳と辞書 辞書検索 [ 開発暫定版 ]
スポンサード リンク

Sabine (crater) : ウィキペディア英語版
Sabine (crater)

Sabine is a lunar crater that forms a nearly matching pair with Ritter to the northwest. The two rims are separated by a distance of only a couple of kilometers. To the west is the bowl-shaped crater Schmidt, and farther to the north are Manners and Arago.
The outer rim of this crater is roughly circular and relatively featureless. The interior floor has a pair of small craterlets and a central rise. There is a ridge at the western edge of the floor that is concentric with the inner wall.
About 85 km to the east-southeast is 'Statio Tranquillitatis' (Tranquility Base), the landing site of the Apollo 11 mission and the first human beings to step on the Moon.
Ranger 8 flew over Sabine prior to impact in Mare Tranquilitatis.
Both Sabine and Ritter were originally believed to be calderas rather than impact craters. In ''To A Rocky Moon'', lunar geologist Don E. Wilhelms summarized: "They are identical twins in morphology and size (29-30 km). They lack radial rim ejecta and secondary craters despite their apparent youth. They are positioned at the presumably active edge of a mare. They are even aligned along graben, the Hypatia rilles. Most significant, they lack deep floors recognized since the days of Gilbert as diagnostic of impacts." However, after the Apollo landings were complete, it was realized that "all craters inside basins suffer enhanced isostatic uplift," because "the thin crust and greater heat inside basins lower the viscosity of the craters' substrate, allowing it to reach isostasy with its surroundings more quickly than can other craters."〔To a Rocky Moon: A Geologist's History of Lunar Exploration. Don E. Wilhelms, University of Arizona Press (1993). ISBN 978-0816510658〕
==Satellite craters==
By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Sabine.
The following craters have been renamed by the IAU, after the three astronauts of Apollo 11.〔Lunar Chart Series (LAC-60 Julius Caesar ), Lunar and Planetary Institute〕
* Sabine B — ''See'' Aldrin.
* Sabine D — ''See'' Collins.
* Sabine E — ''See'' Armstrong.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Sabine (crater)」の詳細全文を読む



スポンサード リンク
翻訳と辞書 : 翻訳のためのインターネットリソース

Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.